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Water in the terrestrial planet-forming zone of the PDS 70 disk - Nature

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Water in the terrestrial planet-forming zone of the PDS 70 disk - Nature

Terrestrial and sub-Neptune planets are expected to form in the inner (less than 10 au) regions of protoplanetary disks1. Water plays a key role in their formation2–4, although it is yet unclear whether water molecules are formed in situ or transported from the outer disk5,6. So far Spitzer Space Telescope observations have only provided water luminosity upper limits for dust-depleted inner disks7, similar to PDS 70, the first system with direct confirmation of protoplanet presence8,9.

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Water in the terrestrial planet-forming zone of the PDS 70 disk - Nature

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